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|description= Airglow correction of WD 1647+375 of the deep exposure where the raw spectrum and the best-fitting airglow template are shown in black and red, respectively. The airglow-corrected spectrum is shown in blue and arbitrarily shifted in flux for clarity. The strong absorption lines of Si ii and O i affected by the airglow are marked in the plot. The dashed black line shows the average continuum flux in the wavelength region 1300–1309 Å. |
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|date=2025-10-28 |
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|source=https://academic.oup.com/mnras/article/543/1/223/8255944#532074368 |
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|author=Snehalata Sahu , Boris T Gänsicke , Jamie T Williams , Detlev G Koester , Jay Farihi , Steven J Desch , Nicola Pietro Gentile Fusillo , Dimitri Veras , Sean N Raymond , Maria Teresa Belmonte |
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== {{int:license-header}} == |
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{{self|cc-by-sa-4.0}} |
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Latest revision as of 12:41, 6 February 2026
| Description |
Airglow correction of WD 1647+375 of the deep exposure where the raw spectrum and the best-fitting airglow template are shown in black and red, respectively. The airglow-corrected spectrum is shown in blue and arbitrarily shifted in flux for clarity. The strong absorption lines of Si ii and O i affected by the airglow are marked in the plot. The dashed black line shows the average continuum flux in the wavelength region 1300–1309 Å. |
|---|---|
| Source |
https://academic.oup.com/mnras/article/543/1/223/8255944#532074368 |
| Date |
2025-10-28 |
| Author |
Snehalata Sahu , Boris T Gänsicke , Jamie T Williams , Detlev G Koester , Jay Farihi , Steven J Desch , Nicola Pietro Gentile Fusillo , Dimitri Veras , Sean N Raymond , Maria Teresa Belmonte |
| Permission (Reusing this file) |
See below. |
I, the copyright holder of this work, hereby publish it under the following license:
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 12:39, 6 February 2026 |  |
1,323 × 901 (417 KB) | Вики-Персик (talk | contribs) |
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